M. Munch

activity

20152020

^{11} B (p, 3 α) γ

reaction at

E_{p} = 0.5 - 2.7

MeV

4 citations · 4 across the 2 of their papers we have counts for

collaborators

3 papers

nucl-ex2020★ 4 cited

Experimental study of the $^{11} B (p, 3 α) γ$ reaction at $E_{p} = 0.5 - 2.7$ MeV

Oliver S. Kirsebom, Alan M. Howard, Michael Munch +3

Our understanding of the low-lying resonance structure in $^{12}$ C remains incomplete. We have used the $^{11} B (p, 3 α) γ$ reaction at proton energies of $E_{p} = 0.5 - 2.7$ MeV as a…

nucl-ex2019

Resolving the 11B(p, $α_{0}$ ) Cross Section Discrepancies between 0.5 and 3.5 MeV

Michael Munch, Oliver Sølund Kirsebom, Jacobus Andreas Swartz +1

The reaction 11B(p, 3 $α$ ) is relevant for fields as diverse as material science, nuclear structure, nuclear astrophysics, and fusion science. However, for the channel proceeding vi…

nucl-ex2015

The 23Na(α,p) 26Mg reaction rate at astrophysically relevant energies

A. M. Howard, M. Munch, H. O. U. Fynbo +4

The production of 26 Al in massive stars is sensitive to the 23 Na(a,p) 26 Mg cross section. Recent experimental data suggest the currently recommended cross sections are underesti…

Experimental study of the 11B(p,3α)γ reaction at Ep​=0.5−2.7 MeV

Resolving the 11B(p, α0​) Cross Section Discrepancies between 0.5 and 3.5 MeV

The 23Na(α,p) 26Mg reaction rate at astrophysically relevant energies

Experimental study of the $^{11} B (p, 3 α) γ$ reaction at $E_{p} = 0.5 - 2.7$ MeV

Resolving the 11B(p, $α_{0}$ ) Cross Section Discrepancies between 0.5 and 3.5 MeV